Compressible Fluids

1918 ◽  
Vol 22 (92) ◽  
pp. 255-257 ◽  
Author(s):  
G. H. Bryan

The average orthodox mathematician who writes or reads books about hydrodynamics is so keen about getting a peg on which he can hang what he calls examples that he quite forgets to apply his formulae to compressible fluids. It appeared to me on reading Colonel De Villamil's letter that a useful purpose would be served by writing the present note; it contains nothing but what anyone could write out for himself, but it was only recently that I made the attempt myself and I should be surprised if many readers have seen the same thing before. We know that in the irrotational motion of an incompressible fluid the velocity potential satisfies Laplace's equation, the present object is to find the corresponding equation for a compressible fluid, to grind it out at full length, and (what is more important than grinding it out) to interpret the result.

1945 ◽  
Vol 7 (2) ◽  
pp. 81-82
Author(s):  
E. T. Copson

The functionis, as is well-known, a general solution of Laplace's equation of degree −1 in (x, y, z). In 1926* I proved that the particular solution r−1Q0 (z/r) cannot be represented in this form whereas the solution r−1Q0 (y/r) can. In the present note I find a very simple expression for the latter solution in the form (1.1), and I deduce from it an apparently new integral formula for Qn (cos θ).


This is the second of two papers dealing with a systematic study of the linearized problems in magneto-hydrodynamics of incompressible and compressible fluids. The first paper (Banos 1955) deals mainly with the general theory of plane homogeneous waves and of time harmonic cylindrical waves propagating in a homogeneous and isotropic conducting fluid of infinite extent embedded in a uniform field of magnetic induction. The medium is assumed to consist of an ideal fluid devoid of viscosity and expansive friction, which is characterized (in rationalized mks units) by the rigorously constant macroscopic parameters p, e and o, where pe = c-2 and o is the (ohmic) conductivity. The present paper deals with the application of the general theory to the determination of the modes of propagation and to the computation of the corresponding propagation constants. It is shown that an incompressible fluid sustains two types of modes: one type devoid of pressure fluctuations (velocity modes), and the other accompanied by pressure oscillations (pressure modes). In the case of cylindrical waves in an incompressible fluid there are two distinct pressure modes, one of which, however, is highly attenuated and therefore of little physical interest. It is found that a compressible fluid also sustains the same class of velocity modes (devoid of pressure fluctuations and hence independent of the velocity of sound in the medium) as an incompressible fluid. In addition, a compressible fluid is shown to propagate two distinct pressure modes which, under appropriate limiting conditions peculiar to each type, behave respectively as a modified sound wave and as a modified magneto-hydrodynamic wave. And, for every mode discussed here, there are presented the limiting forms of the propagation constant in three cases of physical interest: infinite conductivity, slightly attenuated modes, and weak magneto-hydrodynamic coupling which arises when the externally applied field is vanishingly small.


As a result of earlier work by G. I. Taylor on the two-dimensional motion of a compressible fluid, it appears evident that the elastic property of a fluid places a limitation upon the maximum velocity which can exist in a field in order that a certain type of irrotational motion may continue to be possible. So far a complete solution of the equation of motion of a compressible fluid in any particular problem has eluded the workers on this subject, and the greatest theoretical advance came when Taylor used the idea of expanding the velocity potential in a power series about the point of maximum velocity.


1963 ◽  
Vol 3 (1) ◽  
pp. 99-103 ◽  
Author(s):  
P. E. Lush

It is known that various cases of the steady isentropic irrotational motion of a compressible fluid are expressible as variational principle [1], [5]. in particular, the aerofoil problem i.e. the case of plane flow in which a uniform stream is locally deflected, without circulation, by a bounded obstacle, can be expressed in such a form. Thus we make stationary where the region R is that bounded internally by the obstacle (C0) and externally by a circle (CR) of radius R. In this expression φ∞ is the velocity potential for a uniform stream, and φ0 is the velocity potential for the corresponding incompressible flow.


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